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Asymptotically Flat Structure of Hypergravity in Three Spacetime CECS-PHY-15/03 Asymptotically flat structure of hypergravity in three spacetime dimensions Oscar Fuentealba,a;b Javier Matulich,a Ricardo Troncoso,a aCentro de Estudios Científicos (CECs), Av. Arturo Prat 514, Valdivia, Chile. bDepartamento de Física, Universidad de Concepción, Casilla 160-C, Concepción, Chile. E-mail: [email protected], [email protected], [email protected] Abstract: The asymptotic structure of three-dimensional hypergravity without cosmo- logical constant is analyzed. In the case of gravity minimally coupled to a spin-5=2 field, a consistent set of boundary conditions is proposed, being wide enough so as to accommo- date a generic choice of chemical potentials associated to the global charges. The algebra of the canonical generators of the asymptotic symmetries is given by a hypersymmetric nonlinear extension of BMS3. It is shown that the asymptotic symmetry algebra can be recovered from a subset of a suitable limit of the direct sum of the W(2;4) algebra with its hypersymmetric extension. The presence of hypersymmetry generators allows to construct bounds for the energy, which turn out to be nonlinear and saturate for spacetimes that admit globally-defined “Killing vector-spinors”. The null orbifold or Minkowski spacetime can then be seen as the corresponding ground state in the case of fermions that fulfill pe- riodic or antiperiodic boundary conditions, respectively. The hypergravity theory is also explicitly extended so as to admit parity-odd terms in the action. It is then shown that the asymptotic symmetry algebra includes an additional central charge, being proportional to the coupling of the Lorentz-Chern-Simons form. The generalization of these results in the case of gravity minimally coupled to arbitrary half-integer spin fields is also carried out. 1 The hypersymmetry bounds are found to be given by a suitable polynomial of degree s + 2 arXiv:1508.04663v2 [hep-th] 4 Nov 2015 in the energy, where s is the spin of the fermionic generators. Contents 1 Introduction1 2 General Relativity minimally coupled to a spin-5=2 field2 3 Unbroken hypersymmetries: Killing vector-spinors4 3.1 Cosmological spacetimes and solutions with conical defects4 4 Asymptotically flat behaviour and the hyper-BMS3 algebra6 4.1 Flat limit of the asymptotic symmetry algebra from the case of negative cosmological constant 10 5 Hypersymmetry bounds 12 6 Hypergravity reloaded 13 7 General Relativity minimally coupled to half-integer spin fields 15 7.1 Killing tensor-spinors 16 7.2 Asymptotically flat structure and hypersymmetry bounds 17 8 Final remarks 20 A Conventions 24 B Killing vector-spinors from an alternative approach 24 1 C Hyper-Poincaré algebra with fermionic generators of spin n + 2 26 D Asymptotic hypersymmetry algebra 26 D.1 Spin-3=2 fields (supergravity) 26 D.2 Spin-7=2 fields 27 D.3 Spin-9=2 fields 29 1 Introduction It has been shown that the inconsistencies arising in the minimal coupling of a mass- less spin-5=2 field to General Relativity [1], [2], [3], [4] can be successfully surmounted in three-dimensional spacetimes [5]. This theory is known as hypergravity, and it has been recently reformulated as a Chern-Simons theory of a new extension of the Poincaré group with fermionic generators of spin 3=2 [6]. In the case of negative cosmological constant, additional spin-4 fields are required by consistency [7], [8], [9], and it can be seen that – 1 – the anticommutator of the generators of the asymptotic hypersymmetries, associated to fermionic spin-3=2 parameters, leads to interesting nonlinear bounds for the bosonic global charges of spin 2 and 4 [9]. The bounds saturate provided the bosonic configurations ad- mit globally-defined “Killing vector-spinors”. One of the main purposes of this paper is to show how these results extend to the case of asymptotically flat spacetimes in hypergravity, also in the case of arbitrary half-integer spin fields. In the next section we briefly sum- marize the formulation of hypergravity as a Chern-Simons theory for the hyper-Poincaré group in the simplest case of fermionic spin-5=2 fields, while section3 is devoted to explore the global hypersymmetry properties of cosmological spacetimes and solutions with coni- cal defects. In the case of fermions that fulfill periodic boundary conditions, it is shown that the null orbifold possesses a single constant Killing vector-spinor. Analogously, for antiperiodic boundary conditions, Minkowski spacetime is singled out as the maximally (hyper)symmetric configuration, and the explicit expression of the globally-defined Killing vector-spinors is found. The asymptotically flat structure of hypergravity in three space- time dimensions is analyzed in section4, where a precise set of boundary conditions that includes “chemical potentials” associated to the global charges is proposed. The algebra of the canonical generators of the asymptotic symmetries is found to be given by a suitable hypersymmetric nonlinear extension of the BMS3 algebra. It is also shown that this alge- bra corresponds to a subset of a suitable Inönü-Wigner contraction of the direct sum of the W(2;4) algebra with its hypersymmetric extension W 5 . The hypersymmetry bounds (2; 2 ;4) that arise from the anticommutator of the fermionic generators are found to be nonlinear, and are shown to saturate for spacetimes that admit unbroken hypersymmetries, like the ones aforementioned. This is explicitly carried out in section5. In section6, the previous analysis is performed in the case of an extension of the hypergravity theory that includes additional parity-odd terms in the action. It is found that the asymptotic symmetry alge- bra admits an additional central charge along the Virasoro subgroup. The results are then extended to the case of General Relativity minimally coupled to half-integer spin fields in section7, including the asymptotically flat structure, and the explicit expression of the Killing tensor-spinors. The hypersymmetry bounds are shown to be described by a poly- nomial of degree s + 1=2 in the energy, where s is the spin of the fermionic generators. We conclude in section8 with some final remarks, including the extension of these results to the case of hypergravity with additional parity-odd terms and fermions of arbitrary half-integer spin. The coupling of additional spin-4 fields is also addressed. AppendixA is devoted to our conventions, and in appendixB, an alternative interesting form to obtain the explicit form of the Killing vector-spinors is presented. The general form of the hyper-Poincaré algebra is discussed in appendixC, while appendixD includes the asymptotic hypersym- metry algebra in the case of fermionic fields of spin 3=2 (supergravity), as well as for fields of spin 7=2 and 9=2. 2 General Relativity minimally coupled to a spin-5=2 field It has been recently shown that the hypergravity theory of Aragone and Deser [5] can be reformulated as a gauge theory of a suitable extension of the Poincaré group with fermionic – 2 – spin-3=2 generators [6]. The action is described by a Chern-Simons form, so that the dreibein, the (dualized) spin connection, and the spin-5=2 field correspond to the compo- nents of a gauge field given by a a α a A = e Pa + ! Ja + a Qα ; (2.1) a that takes values in the hyper-Poincaré algebra, being spanned by the set fPa;Ja;Qαg. a The fermionic fields and generators are assumed to be Γ-traceless, i. e., Γ a = 0, and a Q Γa = 0, so that the nonvanishing (anti)commutation rules read c c [Ja;Jb] = "abcJ ; [Ja;Pb] = "abcP ; 1 β c [Ja;Qαb] = (Γa) Qβb + "abcQ ; (2.2) 2 α α n o 2 5 1 Qa ;Qb = − (CΓc) P ηab + "abcC P + (CΓ(a) P b) ; α β 3 αβ c 6 αβ c 6 αβ where C stands for the charge conjugation matrix. The Majorana conjugate then reads ¯ β αa = a Cβα. Since the algebra admits an invariant bilinear form, whose only nonvanishing components are given by D a b E 2 ab 1 abc hJa;Pbi = ηab ; Q ;Q = Cαβη − " (CΓc)αβ ; (2.3) α β 3 3 the action can be written as k 2 I [A] = AdA + A3 ; (2.4) 4π ˆ 3 which up to a surface term reduces to k a ¯ a I = 2R ea + i aD : (2.5) 4π ˆ a a 1 abc Here R = d! + 2 " !b!c is the dual of the curvature two-form, and since the fermionic field is Γ-traceless, its Lorentz covariant derivative fulfills 1 D a = d a + !bΓ a + "abc! 2 b b c a 3 b a a b = d + ! Γb − !bΓ : (2.6) 2 The field equations are then given by F = dA + A2 = 0, whose components read a a 3 ¯ a b a R = 0 ;T = i bΓ ; D = 0 ; (2.7) 4 where T a = Dea corresponds to the torsion two-form. Therefore, by construction, the action changes by a boundary term under local hy- α a persymmetry transformations spanned by δA = dA + [A; λ], with λ = a Qα, so that the transformation law of the fields reduces to a 3 a b a a a δe = i¯bΓ ; δ! = 0 ; δ = D : (2.8) 2 Note that the transformation rules of the fields in [5] agree with the ones in (2.8), on-shell. – 3 – 3 Unbroken hypersymmetries: Killing vector-spinors It is interesting to explore the set of bosonic solutions that possess unbroken global hy- persymmetries. According to the transformation rules of the fields in (2.8), this class of configurations has to fulfill the following Killing vector-spinor equation: a 1 b a abc d + ! Γb + " !bc = 0 ; (3.1) 2 where the spin-3=2 parameter a is Γ-traceless.
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